1 / 40

Enceladus Life Finder Mission

Enceladus Life Finder Mission. 16 November 2016. Io Europa Enceladus. All these moons are heated by tides that stretch and press them. Enceladus. Size: 513.2 × 502.8 × 496.6 km Composition: ice and rock Jets – source of Saturn ’ s E-ring Habitability:

khurdle
Télécharger la présentation

Enceladus Life Finder Mission

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Enceladus Life FinderMission 16 November 2016

  2. Io Europa Enceladus All these moons are heated by tides that stretch and press them

  3. Enceladus • Size: 513.2 × 502.8 × 496.6 km • Composition: ice and rock • Jets – source of Saturn’s E-ring Habitability: • Enceladus ejects plumes of salt water + grains of silica-rich sand, nitrogen (in ammonia), nutrients and organic molecules • This indicates that hydrothermal activity—an energy source—may be at work in Enceladus's subsurface ocean. • The underground warm water provides a possible location for life, perhaps similar to that found under the ice cover of Antarctic lakes.

  4. Enceladus Surface • Voyager images (1980,1981) showed both heavily cratered and smooth regions • Cassini saw great fractures in the south, called ‘tiger stripes’ • These cracks probably extend down to water reservoirs, because ice grains and vapor jet out of them • These are the warmest parts of Enceladus surface

  5. Enceladus Interior • Differentiated: Rocky core at the center, surrounded by ice mantle, with water oceans and seas, covered by a cold, icy crust • Some unknown plumbing brings the water under pressure to the surface, where it freezes and shoots out like an ice cannon • Thus the jets can sample the interior without needing to land and drill down

  6. ISS observation of jets

  7. “Tiger stripes”

  8. Cryovolcanism

  9. Tiger Stripes

  10. IR images • -> Temperature: • Tiger Stripes • are warm • Source of heat? • Tidal heating • Radioactive heating • Chemistry (ammonia)

  11. Tiger Stripes close-up

  12. Even closer!

  13. Discussion Topic: Talk with those near you • What types of experiments would you carry to Enceladus to look for life? How are these similar or different from those for Europa?

  14. Future Search for Enceladus Life • First: Where is the water? • At South Pole tiger stripes • 1-50km deep • Getting to Enceladus is not easy, it is a long trip, requires multiple rocket burns to reach it and to land softly • How to reach water • Fly through plumes • Land safely near the plume (not easy because the surface is rough) and then drill (hot brick?) • Staged approach • Saturn orbiter with multiple flybys provides detailed maps; then an Enceladus orbiter and lander; finally, mobility to explore with a rover • Tests for life • Microscopy, culture a sample, labeled nutrients, identify life molecules: amino acids, polypeptides, polysaccharides, lipids, nucleic acids and DNA

  15. Summary • Enceladus is heated by tides • Water erupts in jets to form a giant plume • This shows a salty, underground ocean • Enceladus has all the requirements for life • Liquid water, biogenic elements from rocks and meteorites, energy from sunlight and geothermal • Search for life by flying through and by drilling down to the ocean

More Related